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What is Periodic Optical Variability in Blazar S5 0716+714 about?

This study investigates periodic oscillations in the intra-day optical light curves of the blazar S5 0716+714 using wavelet analysis on 20 selected light curves. The findings reveal strong candidates for quasi-periodic variations, suggesting that some variability in blazars may be linked to accretion disk fluctuations, with implications for estimating the mass of the central black hole. The research highlights the complexity of emission mechanisms in blazars, as no correlation was found between flux levels

Author

travylyyf

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EN